Published November 1976 | Version v1
Journal article

The height variation of granular and oscillatory velocities

  • 1. Sacramento Peak Observatory, Air Force Geophysics Laboratory, Sunspot, N.M. 88349, USA

Description

Previous observations of spatially-resolved vertical velocity variations in ten lines of Fe I spanning the height range 0 < approximately h < approximately 1000 km are re-analyzed using velocity weighting functions. The amplitudes and scale heights of granular and oscillatory velocities are determined, as well as those of the remaining unresolved velocities. It is found that the optimal representation of the amplitude of the outward-decreasing granular velocities is an exponentially decreasing function of height, with a scale height of 150 km and a velocity at zero height of 1.27 km s-1. The optimal representation of the same quantities for oscillatory velocities is an exponential increase with height, with a scale height of 1100 km and a velocity at zero height of 0.35 km s-1. The remaining unresolved velocities decrease with height, with a scale height of 380 km and a velocity at zero height of 2.3 km s-1. (Auth.)

Part of:
Vertical phase variation and mechanical flux in the solar 5-minute oscillation

Additional details

Identifiers

Publishing Information

Journal Title
Solar Physics
Journal Volume
50
Journal Issue
2
Series
Sol. Phys.
Journal Page Range
239-254
ISSN
0038-0938

Optional Information

Notes
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